Ana C. O. Leite
Forthcoming high-resolution ultra-stable spectrographs will play an important role in the quest for new physics, by enabling a new generation of precision consistency tests and complementing other facilities in terms of redshift coverage. We discuss an example of this synergy, by quantifying (through various figures of merit) improvements in dark energy constraints obtained by combining measurements of fundamental couplings with Type Ia supernovae from Euclid and the ELTs.
2013 October 30, 13:30
Centro de Astrofísica da Universidade do Porto (Classroom)
Rua das Estrelas, 4150-762 Porto